Observer-Sun Angles. ), Solar altitude angle (α s. ) and solar azimuth angle (γ s )). θ z. = 90 o α s

Transcription

1 Observer-Sun Angles Direction of Beam Radiation: The geometric relationships between a plane of any particular orientation relative to the earth at any time and the incoming beam solar radiation can be described in terms of several angles (Latitude(φ), Declination(δ), Slope(β), Surface azimuth angle(γ), Hour angle(ω), Angle of incidence(θ), Zenith angle(θ z ), Solar altitude angle (α s ) and solar azimuth angle (γ s )). θ z = 90 o α s

2 Sun s Position Zenith ψ α ψ ψ sinα = sinδ sinφ + cosδ cosω cosψ = sinα sinφ sinδ cosα cosω

3 Observer-Sun Angles Source: Photovoltaic systems Engineering by Messenger & Ventre, CRC 2000.

4 Collector Angle There is a set of useful relationships among these angles. Equations relating the angle of incidence of beam radiation on a surface, θ, to the other angles are: δ = 23.45sin n β 365 equator 90 o cosθ =sinδ sinφ cosβ and sinδ cosφ sinβ cosγ +cosδ cosφ cosβ cosω +cosδ sinφ sinβ cosγ cosω +cosδ sinβ sinγ sinω cosθ =cosθ z cosβ +sinθ z sinβ cos(γ s γ) For horizontal surfaces. The angle of incidence is the zenith angle of the sun θ z ( 0 o or 90 o when the sun is above the horizon). For this situation β=0 cosθ z =cosθ cosδ cosω +sinθ sinδ Beam radiation θ normal β

5 The optimum tilt angle for a south facing photovoltaic module in Tallahassee (latitude, φ = N) at solar noon on March 1. March 1 - sixtieth day of the year Solar declination δ = 23.45sin n 365 Tilt Angle of a PV Module ( ) = 23.45sin 360 ( ) ) = -8.3 o 365 Tilt angle: φ δ = o

6 Tracking Surface Angles For a plane rotated about a horizontal east-west axis with single daily adjustment of beam radiation being normal to the surface at noon each day: cosθ = sin 2 δ + cos 2 δ cosω The slope of the surface is fixed for each day: β = φ δ If (φ - δ) >0, γ = 0 o ; (φ - δ) < 0, γ = 180 o At solar noon φ z = φ - δ

7 Sunset Hour Angle The sunset hour angle ω s, when θ z = 90 is given by cosω = s sinφ sinδ = tanφ tanδ cosφ cosδ Number of daylight hours: If latitude and declination are known, the day length can be calculated from the formula: N 2 = cos 1 15 ( tanφ tanδ ) ω = 12 T o Where T is the time of day expressed with respect to solar midnight on a 24 hr clock.

8 Nomogram Information on latitude (φ) and declination (δ) leads directly to times of sunset and day length for either hemisphere. These parameters can be conveniently determined from the nomogram (shown on the side) as devised by Whillier (1965b).

9 Sunshine Days

10 Radiation on Horizontal Surface Extraterrestrial radiation on a horizontal surface: This is defined as the theoretically possible radiation (G o ) that would be available if there were no atmosphere. G o 360n = Gsc cos ( cosφ cosδ cosω sinφ sinδ ) G SC is the solar constant and n is the day of the year.

11 Variation of Extraterrestrial Radiation G on 360n = G + sc cos 365 Where G on is the radiation measured on the plane normal to the radiation on the n th day of the year.

12 Radiation on Horizontal Surface The integrated daily (sunrise to sunset) extraterrestrial radiation (H o ) on a horizontal surface is given by: H o 24 x3600g = SC 360n πω + s cos cosφ cosδ sinωs + sin φ sin δ π where G SC is in watts/m 2 ω S, the sunset hour angle, is in degrees H o is in joules/m 2

13 Radiation on Horizontal Surface H o as a function of latitude for the northern and southern hemispheres: Curves are for dates that give the mean radiation for the month Values of H o for any day can be estimated by interpolation.

14 Solar Radiation Data on Horizontal Surface

15 Solar Irradiance In the design of photovoltaic systems the irradiation over one day is of particular significance. Solar irradiance integrated over a period of time is called solar irradiance (total power from a radiant source falling on a unit area). The average daily solar radiation on the ground G av (averaged both over the location and time of the year) can be obtained using the following relationship. G av = h = 5.75kWh /day Where the average irradiance outside the atmosphere = 342 W/m 2 Solar radiation observed on the earth s surface is 30% lower on account of scattering and reflection of radiation.

16 Mean Daily Solar Radiation

17 Solar Radiation Data on Horizontal Surface 1 cal/cm 2 = kj/m 2 ; 1 kwh = 3.6 MJ

18 Solar Radiation in the Atmosphere

19 Tracking Surfaces Angles for Tracking Surfaces: Some solar collectors track the sun by moving in prescribed ways to minimize the angle of incidence of beam radiation on their surfaces and thus maximize the incident beam radiation. Classification of tracking systems by motion: Rotation about a single axis Rotation about two axes The axis described above could have any orientation but is usually horizontal east-west, horizontal north-south, vertical or parallel to the earth s axis. For relationships between the angles of incidence and the surface azimuth angles, refer to the handout.

20 Tilted Surfaces Ratio of Beam radiation on tilted surface to that on horizontal surface (R b ) : The most commonly available data are total radiation for hours and or days whereas the need is for beam and diffuse radiation on the plane of a collector (normally tilted). R b = G b, T G b = G G b, n b, n cosθ cosθ z = cosθ cosθ z For horizontal surfaces: cosθ z =cosθ cosδ cosω +sinθ sinδ

21 Zenith Angle Effect

22 Solar radiation on an inclined surface Step 1: Obtain the site data to determine the separate diffusive and beam contributions to the global irradiation (G) on the horizontal plane. Use the extraterrestrial daily irradiation B o, as a reference and calculate the clearness index K T. This describes the average attenuation of solar radiation by the atmosphere at a given site during a given month. K T = G B o Note: In the evaluation of B o, the variation of the extraterrestrial irradiance on account of the eccentricity of the earth s orbit (~ ± 3%) is taken into account B o = 24 π S cos 2πd n ( 365 cosϕ cosδ sinω s + ω s sinϕ sinδ) S: Solar constant = 1367 W/m 2 ; d n ; number of the day in the year; Latitude(φ), Declination(δ), Sunrise hour angle ω s = cos -1 (-tan φ tan δ) Source: Solar Electricity by Tomas Markvart, Wiley, 2003

23 Solar radiation on an inclined surface Step 2: The diffuse radiation is obtained using the empirical rule that the diffuse fraction is a universal function of clearness index. B: Beam irradiation D: Diffuse irradiation G: Global daily irradiation D G = f ( K T )=1 1.13K T B = G D

24 Solar radiation on an inclined surface Step 3: Appropriate angular dependences of each component are used to determine the diffuse and beam irradiation on the inclined surface. With the allowance for reflectivity of the surrounding area. The total daily irradiation on the inclined surface is obtained by adding the three contributions.

25 Solar radiation on an inclined surface Beam radiation: The beam radiation B(β) on a south-facing panel inclined at an angle β to the horizontal surface is given by B β sin(φ β)sinδ cosφ cosδ sinω s + ω s sinφ sinδ ()= B cos(φ β)cosδ sinω o + ω o ω o = min ω s,ω s ' ω s ' { } = cos 1 { tan(φ β)tanδ} Where ω s and ω s are the sunrise angle above the horizon and the sunrise angle above a plane inclined at an angle β to the horizontal

26 Solar radiation on an inclined surface Diffusive radiation: Assuming it is distributed isotropically over the sky dome, the diffusive radiation on the inclined surface is given by D β ()= 1 2 Albedo (ground reflected) radiation: It is generally small and a simple isotropic model is sufficient as given below. R β ()= 1 2 ρ Is the reflectivity of the ground. ( 1+ cosβ)d ( 1+ cosβ)ρg

27 Total Global irradiation: Solar radiation on an inclined surface G β ( )= B β ( )+ D β ( )+ R β ( )

28 Solar radiation on an inclined surface Daily irradiation in Barcelona

29 Solar radiation on an inclined surface South Facing

30 Shading Effects Problems associated with Shading: Collectors or other receivers by near-by trees, buildings etc. Shading of collectors in subsequent rows other than the first row in a multi-row array. Shading of windows by overhangs and wingwalls.

31 Shading Effects Estimating the amount of time the sun is obscured by an obstruction: Calculate the object azimuth angle (γ o ) and the object altitude angle (α o ). Note that the object is the cause of shading. Locate these angular co-ordinates on the Solar plot and join by a smooth curve. Estimate the amount of time the Sun is obscured.

32 Shading Effects Shading due to overhangs and wingwalls: Architectural features like overhangs and wingwalls shade windows from beam radiation. The solar position charts can be used to determine when points on the receiver are shaded.

33 Shading Effects Shading due to multi-row array of collectors: In a multi-row collector array, the first row is unobstructed, but subsequent rows may be partially shaded as shown.

34 Shading Effects Effect of Profile angle on shading due to multi-row array of collectors: The Profile angle is the angle through which a plane that is initially horizontal must be rotated about an axis in the plane of the surface in question in order to include the sun. When the collectors are long in extent so the end effects are negligible, the profile angle provides a useful means of determining shading. Referring to the previous slide, if the profile angle is greater than angle CAB, no point on row N will be shaded by row M. On the contrary, if the profile angle is less than angle CAB, the portion of row N below point A will be shaded from beam radiation.

35 US Radiation Map Source: NREL